Galactic and interplanetary cosmic rays relevant for LISA test-mass charging

C. Grimani; M. Fabi; R. Stanga; L. Marconi

doi:10.1063/1.2405040

Galactic and interplanetary cosmic rays relevant for LISA test-mass charging

C. Grimani
, M. Fabi
, R. Stanga
, L. Marconi

University of Urbino Carlo Bo
Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
University of Florence

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

Galactic (GCR) and solar cosmic rays with energies larger than 100 MeV(/n) penetrate and charge the test masses of the LISA missions. Spurious forces between the test-masses and the surrounding electrodes might be mistaken for genuine gravitational wave signals. In this paper, we report about galactic and interplanetary cosmic rays charging the LISA test-masses as a function of the solar activity level and Global Solar Magnetic Field (GSMF) polarity. The simulation work has been carried out with the use of the Fluka Monte Carlo program (2005 release) and completes our previous results on galactic cosmic rays.

langue originale	Anglais
Pages (de - à)	184-188
Nombre de pages	5
journal	AIP Conference Proceedings
Volume	873
Les DOIs	https://doi.org/10.1063/1.2405040
état	Publié - 27 déc. 2006
Modification externe	Oui

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10.1063/1.2405040

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title = "Galactic and interplanetary cosmic rays relevant for LISA test-mass charging",

abstract = "Galactic (GCR) and solar cosmic rays with energies larger than 100 MeV(/n) penetrate and charge the test masses of the LISA missions. Spurious forces between the test-masses and the surrounding electrodes might be mistaken for genuine gravitational wave signals. In this paper, we report about galactic and interplanetary cosmic rays charging the LISA test-masses as a function of the solar activity level and Global Solar Magnetic Field (GSMF) polarity. The simulation work has been carried out with the use of the Fluka Monte Carlo program (2005 release) and completes our previous results on galactic cosmic rays.",

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author = "C. Grimani and M. Fabi and R. Stanga and L. Marconi",

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day = "27",

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AU - Grimani, C.

AU - Fabi, M.

AU - Stanga, R.

AU - Marconi, L.

PY - 2006/12/27

Y1 - 2006/12/27

N2 - Galactic (GCR) and solar cosmic rays with energies larger than 100 MeV(/n) penetrate and charge the test masses of the LISA missions. Spurious forces between the test-masses and the surrounding electrodes might be mistaken for genuine gravitational wave signals. In this paper, we report about galactic and interplanetary cosmic rays charging the LISA test-masses as a function of the solar activity level and Global Solar Magnetic Field (GSMF) polarity. The simulation work has been carried out with the use of the Fluka Monte Carlo program (2005 release) and completes our previous results on galactic cosmic rays.

AB - Galactic (GCR) and solar cosmic rays with energies larger than 100 MeV(/n) penetrate and charge the test masses of the LISA missions. Spurious forces between the test-masses and the surrounding electrodes might be mistaken for genuine gravitational wave signals. In this paper, we report about galactic and interplanetary cosmic rays charging the LISA test-masses as a function of the solar activity level and Global Solar Magnetic Field (GSMF) polarity. The simulation work has been carried out with the use of the Fluka Monte Carlo program (2005 release) and completes our previous results on galactic cosmic rays.

KW - Galactic cosmic rays

KW - Interplanetary cosmic rays

KW - LISA missions

KW - Test-mass charging

UR - https://www.scopus.com/pages/publications/33845658286

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DO - 10.1063/1.2405040

M3 - Article

AN - SCOPUS:33845658286

SN - 0094-243X

VL - 873

SP - 184

EP - 188

JO - AIP Conference Proceedings

JF - AIP Conference Proceedings

ER -

Galactic and interplanetary cosmic rays relevant for LISA test-mass charging

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